Planned stereo pairs have suitable stereo convergence angles and illumination by design.
In addition to planned stereo pairs, the Pairendipity software can identify overlapping
HiRISE images that are serendipitously suitable for stereo processing and find stereo
pairs within the CTX dataset.
Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below.
Since this list is based on produced stereo anaglyphs it also contains a few serendipitous
pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed
in the “Pairendipity Stereo” link, while CTX stereo pairs are listed
in “Pairendipity CTX Stereo”.
Images taken close together in time minimize illumination and frost differences and are
especially useful (see the Delta-Days column in the Pairendipity files or difference
the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs
with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs.
| Inverted Channels or Possible Eskers in Basin in Northwest Arabia Terra: ESP_090371_2150 ESP_090437_2150 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 34.65 | 6.53 | 8.59 | -5.85 | 57.7 | 59.7 |
| Vent East of Ascraeus Mons: ESP_090375_1925 ESP_090520_1925 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 12.13 | 261. | -5.8 | 10.07 | 56.2 | 55.7 |
| Terrain around Crater in Terra Sabaea: ESP_090409_2165 ESP_090132_2165 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 36.18 | 50.6 | -6.7 | 5.045 | 59.7 | 55.3 |
| Light-Toned Exposures on Floor of Coprates Chasma: ESP_090413_1645 ESP_090136_1645 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -15.3 | 307. | 4.12 | 18.86 | 60.0 | 60.1 |
| Sample of Aprons around Massifs in Erebus Montes: ESP_090404_2185 ESP_090338_2185 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 38.34 | 187. | -8.8 | 5.02 | 60.5 | 58.4 |
| An Inverted Channel in Flammarion Crater: ESP_089631_2065 ESP_090330_2065 (Interval in Earth days: 54) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 26.02 | 48.9 | 5.65 | -12.0 | 49.6 | 57.2 |
| Deep in Valles Marineris: ESP_089134_1655 ESP_088633_1655 (Interval in Earth days: 39) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -14.3 | 303. | -5.3 | -18.1 | 64.4 | 65.7 |
| Inverted Channel in Noachis Terra: ESP_090252_1600 ESP_090397_1600 (Interval in Earth days: 12) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -19.8 | 23.1 | -5.0 | 18.55 | 63.1 | 60.5 |
| Light-Toned Exposures in Capri Chasma: ESP_090215_1670 ESP_090149_1670 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -12.9 | 312. | -3.4 | 16.26 | 60.6 | 59.3 |
| Mesas in Arcadia Planitia: ESP_090180_2265 ESP_090325_2265 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 46.27 | 179. | 0.44 | 14.76 | 58.9 | 59.9 |
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